The MeerKAT Absorption Line Survey
     
The MALS utilizes excellent point-source sensitivity and frequency coverage of the MeerKAT telescope to carry out the most sensitive seeach of HI 21-cm and OH 18-cm lines at 0<z<2.  The survey will be carried out using the L-band (900-1670 MHz) and UHF-band (580-1015 MHz) receivers. The detailed survey design is available at:

http://adsabs.harvard.edu/abs/2017arXiv170807371G






 
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